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Home All issues A&A, 439 2 (2005) 627-633 Article references

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Cited article:

ATOMIUM: Probing the inner wind of evolved O-rich stars with new, highly excited H2O and OH lines

A. Baudry, K. T. Wong, S. Etoka, et al.
Astronomy & Astrophysics 674 A125 (2023)
https://doi.org/10.1051/0004-6361/202245193

A HIFI view on circumstellar H2O in M-type AGB stars: radiative transfer, velocity profiles, and H2O line cooling

M. Maercker, T. Danilovich, H. Olofsson, et al.
Astronomy & Astrophysics 591 A44 (2016)
https://doi.org/10.1051/0004-6361/201628310

Detailed modelling of the circumstellar molecular line emission of the S-type AGB star W Aquilae

T. Danilovich, P. Bergman, K. Justtanont, et al.
Astronomy & Astrophysics 569 A76 (2014)
https://doi.org/10.1051/0004-6361/201322807

Interstellar Water Chemistry: From Laboratory to Observations

Ewine F. van Dishoeck, Eric Herbst and David A. Neufeld
Chemical Reviews 113 (12) 9043 (2013)
https://doi.org/10.1021/cr4003177

MAGNETIC FIELDS IN EVOLVED STARS: IMAGING THE POLARIZED EMISSION OF HIGH-FREQUENCY SiO MASERS

W. H. T. Vlemmings, E. M. L. Humphreys and R. Franco-Hernández
The Astrophysical Journal 728 (2) 149 (2011)
https://doi.org/10.1088/0004-637X/728/2/149

CIRCUMSTELLAR ION-MOLECULE CHEMISTRY: OBSERVATIONS OF HCO+IN THE ENVELOPES OF O-RICH STARS AND IRC+10216

R. L. Pulliam, J. L. Edwards and L. M. Ziurys
The Astrophysical Journal 743 (1) 36 (2011)
https://doi.org/10.1088/0004-637X/743/1/36

A chemical inventory of the S-type AGB starχ Cygni based onHerschel/HIFI observations of circumstellar line emission

F. L. Schöier, M. Maercker, K. Justtanont, et al.
Astronomy & Astrophysics 530 A83 (2011)
https://doi.org/10.1051/0004-6361/201116597

THE MASS-LOSS RETURN FROM EVOLVED STARS TO THE LARGE MAGELLANIC CLOUD. II. DUST PROPERTIES FOR OXYGEN-RICH ASYMPTOTIC GIANT BRANCH STARS

Benjamin A. Sargent, S. Srinivasan, M. Meixner, et al.
The Astrophysical Journal 716 (1) 878 (2010)
https://doi.org/10.1088/0004-637X/716/1/878

A HIFI preview of warm molecular gas aroundχCygni: first detection of H2O emission toward an S-type AGB star

K. Justtanont, L. Decin, F. L. Schöier, et al.
Astronomy and Astrophysics 521 L6 (2010)
https://doi.org/10.1051/0004-6361/201015092

Water content and wind acceleration in the envelope around the oxygen-rich AGB star IK Tauri as seen byHerschel/HIFI

L. Decin, K. Justtanont, E. De Beck, et al.
Astronomy and Astrophysics 521 L4 (2010)
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Circumstellar water vapour in M-type AGB stars: constraints from H$_{\sf 2}$O(1$_{\sf 10}$–1$_{\sf 01}$) lines obtained with Odin

M. Maercker, F. L. Schöier, H. Olofsson, et al.
Astronomy & Astrophysics 494 (1) 243 (2009)
https://doi.org/10.1051/0004-6361:200810017

CARBON CHEMISTRY IN THE ENVELOPE OF VY CANIS MAJORIS: IMPLICATIONS FOR OXYGEN-RICH EVOLVED STARS

L. M. Ziurys, E. D. Tenenbaum, R. L. Pulliam, N. J. Woolf and S. N. Milam
The Astrophysical Journal 695 (2) 1604 (2009)
https://doi.org/10.1088/0004-637X/695/2/1604

A multi-transition submillimeter water maser study of evolved stars. Detection of a new line near 475 GHz

K. M. Menten, A. Lundgren, A. Belloche, S. Thorwirth and M. J. Reid
Astronomy & Astrophysics 477 (1) 185 (2008)
https://doi.org/10.1051/0004-6361:20078349

A Detailed Analysis of the Dust Formation Zone of IRC +10216 Derived from Mid‐Infrared Bands of C2H2and HCN

J. P. Fonfria, J. Cernicharo, M. J. Richter and J. H. Lacy
The Astrophysical Journal 673 (1) 445 (2008)
https://doi.org/10.1086/523882

Circumstellar water vapour in M-type AGB stars: radiative transfer models, abundances, and predictions for HIFI

M. Maercker, F. L. Schöier, H. Olofsson, P. Bergman and S. Ramstedt
Astronomy & Astrophysics 479 (3) 779 (2008)
https://doi.org/10.1051/0004-6361:20078680

Distribution and Kinematics of the HCN (3-2) Emission Down to the Innermost Region in the Envelope of the O-rich Star W Hydrae

Sébastien Muller, Dinh-V-Trung, Jin-Hua He and Jeremy Lim
The Astrophysical Journal 684 (1) L33 (2008)
https://doi.org/10.1086/592110

Observations of the Circumstellar Water \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $1_{10}arrow 1_{01}$ \end{document} and Ammonia \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{! wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $1_{0}arrow 0_{0}$ \end{document} Lines in IRC +10216 by theOdinSatellite

T. I. Hasegawa, S. Kwok, N. Koning, et al.
The Astrophysical Journal 637 (2) 791 (2006)
https://doi.org/10.1086/498561

Circumstellar Atomic Hydrogen in Evolved Stars1

E. Gérard and T. Le Bertre
The Astronomical Journal 132 (6) 2566 (2006)
https://doi.org/10.1086/508811